Memorial Image Taken on Mars on Sept. 11, 2011. This view of an American flag on metal recovered from the site of the World Trade Center towers shortly after their destruction on Sept. 11, 2001, was taken on Mars by NASA’s Opportunity rover on Sept. 11, 2011, the 10th anniversary of the attacks on the towers. Credit: NASA/JPL-Caltech/Cornell University/Arizona State University
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On this somber occasion marking the 10th anniversary of the tragic events of 9/11, NASA’s Opportunity Mars rover has taken new images of itself on 9/11/11 showing a piece of metal recovered from the wreckage of the Twin Towers of the World Trade Center in New York City that was carried all the way to the planet Mars as a commemorative memorial to the innocent victims of the terrorist attacks of Sept 11, 2001.
On Sept. 11, 2011 (Martian Sol 2713), Opportunity snapped the memorial image above showing the Rock Abrasion Tool (RAT) and an American Flag – evoking the memory of the Twin Towers – from a slope on a Martian hill named Cape York which in turn is a segment of the rim of a gigantic crater named Endeavour.
Opportunity is still roving the red planet’s surface, nearly 8 years after safely landing on Jan 24, 2004. After an epic trek she recently arrived at the gigantic 14 mile wide Endeavour crater .
Opportunity took the new image of the RAT and 9/11 US Flag memorial on Mars on the exact day timed to coincide with the 10th anniversary of the attacks.
The image shows the arm extended for inspection of target on a rock called “Chester Lake”, according to NASA officials. Opportunity is driving in a northerly direction up the Cape York hill on her scientific expedition of the crater’s rim.
Memorial Close-up Image Taken on Mars on Sept. 11, 2011
Close-up image taken on 9/11/11 of a piece of metal with the American flag on it of a NASA’s Opportunity rover on Mars is made of aluminum recovered from the site of the World Trade Center towers in the weeks after their destruction on Sept. 11, 2001. Credit: NASA/JPL-Caltech/Cornell University/Arizona State University
Both towers of the World Trade Center in New York City were destroyed by the terrorists on that terrible day and nearly 3000 precious people were killed during horrifying historic events that changed America and the World forever.
The RAT was built for NASA and both rovers by Honeybee Robotics which at that time was located less than a mile away from the WTC near the southern tip of Manhattan.
Steve Gorevan, the founder and chairman of Honeybee and a member of the rover science team, told me in a past interview that he was on his way to work and out on the city streets within a few blocks of the Twin Towers when he suddenly heard the sounds of the jet engines just before the first tower was struck.
Gorevan and the Honeybee employees watched the tragic events unfold from their company’s offices and rooftop the rest of the day. Following the terror attacks, Gorevan said access to Honeybee was restricted for weeks and the firm was on a tight deadline to deliver the RAT’s to NASA and the Jet Propulsion Laboratory in California where the rovers were being assembled.
The idea for somehow placing a Martian memorial on the rovers was presented. Gorevan told me that he was able to secure metallic pieces from the WTC wreckage through the Office of the then NYC Mayor Rudy Guiliani a few weeks after the attacks.
Memorial Image Taken on Mars on Sept. 11, 2011 of Robotic Arm at Work showing US Flag 9/11 Memorial on the Rock Abrasion Tool (RAT). Image taken on Sol 2713 as the robot investigates a rock outcrop called Chester Lake. Credit: NASA/JPL-Caltech
Aluminum shards were delivered by the Mayor’s office to Honeybee along with a note indicating their authenticity. These were soon fashioned into an aluminum shield that was placed on each RAT along with a US Flag. The shield serves as a cable guard.
Gorevan says the twin towers memorial was purposely kept quiet for some time until well after both rovers landed out of respect for the victims’ families.
Opportunity is healthy and continuing her exploration of Endeavour crater which harbors geologic formations and rocks unlike any previously investigated by either of the Mars Exploration (MER) rovers.
Along the rim of Endeavour crater rover scientists hope to discover and analyze clay minerals which formed in pH neutral water billions of years ago and a habitable environment much more favorable to the formation of life compared to all the other spots studied by either rover thus far.
Both rovers far exceeded their original 90 days warranties with many years of added bonus time for science exploration.
Endeavour Crater Panorama from Opportunity, Sol 2681, August 2011
Opportunity arrived at the rim of Endeavour on Sol 2681, August 9, 2011 and climbed up the ridge known as Cape York. Odyssey crater is visible at left. Opportunity drove north from here to snap a new 9/11 memorial image on Sept 11, 2011 marking the 10th anniversary of the 9/11 terrorist attacks.
Mosaic Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer
As we approach the tenth anniversary of the September 11 World Trade Center attacks (has it already been ten years??) countless hearts and minds will be remembering the fateful day our world changed forever, and the many people who tragically lost their lives in the catastrophic collapse of the twin towers. Memorial events will be held in many locations around the world… and even, in a small yet poignant way, on another world. For, unknown to many, two pieces of the World Trade Center are on the surface of Mars: one affixed to the rover Spirit which sits silently in its permanent position near a small plateau called “Home Plate” and the other on its sister rover Opportunity, currently exploring the rim of the vast Endeavour crater.
Much more than scientific exploration tools, these rovers are also interplanetary memorials to the victims of 9/11.
In September of 2001 workers at Honeybee Robotics in lower Manhattan were busy preparing the Rock Abrasion Tools that the twin rovers Spirit and Opportunity would each be equipped with, specialized instruments that would allow scientists to study the interiors of Martian rocks. After the World Trade Center attacks occurred, the company wanted a way to memorialize those who had lost their lives.
Through what was undoubtedly some incredibly skillful use of contacts, Honeybee founder and MER science team member Stephen Gorevan – on a suggestion by JPL engineer Steve Kondos and with help from the NYC mayor’s office and rover mission leader Steve Squyres – was able to procure two pieces of aluminum from the tower debris. These were fashioned into cylindrical cable shields by a contracted metal shop in Round Rock, Texas, and had American flags adhered to each by Honeybee engineer Tom Myrick.
The rovers were launched in the summer of 2003 and have both successfully operated on Mars many years past their planned initial mission timelines. Spirit currently sits silent, having ceased communication in March 2010, but Opportunity is still going strong in its exploration of the Martian surface.
“It’s gratifying knowing that a piece of the World Trade Center is up there on Mars. That shield on Mars, to me, contrasts the destructive nature of the attackers with the ingenuity and hopeful attitude of Americans.”
– Stephen Gorevan, Honeybee Robotics founder and chairman
The image above, taken in 2004, shows the cable shield with American flag on the Rock Abrasion Tool attached to Spirit.
These memorials will remain on Mars long after both rovers have ceased to run, subtle memorials to thousands of lives and testaments to our ability to forge ahead in the name of hopefulness and discovery.
Mars-bound astronauts may require different meals than the ones prepared for the shuttle program. Image Credit: NASA Johnson Space Center (NASA-JSC)
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NASA has made tremendous progress during the past fifty years with regards to food science. Gone are the days of nutrients in toothpaste style tubes and it’s safe to assume NASA astronauts haven’t had to drink Tang in decades.
At a recent meeting of the American Chemical Society, Maya R. Cooper, senior research scientist at NASA’s Space Food Systems Laboratory discussed how feeding astronauts will be one of the most difficult issues to resolve before launching a manned mission to Mars.
Despite all the progress NASA has made, what challenges still need to be overcome to feed the crew of a manned mission to Mars?
When we plan a camping trip, not much thought is given to what will be eaten during a weekend, a week, or even a month’s time. Modern food science has given us products that are safe to eat after even weeks, and in some cases months. It is very easy to go to the store and load up on delicious and nutritious food, with the expectation that said food will be relatively safe to eat with minor concerns for safety.
Manned spaceflight however, isn’t your average camping trip. Even during a one to two week mission, NASA astronauts can’t just open a refrigerator and make themselves a cold-cut sandwich. Food scientists at NASA must specially prepare meals for astronauts in order to ensure said meals are safe to consume during the mission, not only for the crew, but for their habitat as well. The average can or bottle of pop wouldn’t provide the same level of safety and satisfaction for a crew in space as it would for a person on Earth. Food crumbs can clog air filters or become lodged into sensitive equipment. Basically, what works well for a camping trip doesn’t always work for an ISS mission and what works for the ISS crew may not work for a multi-year mission to Mars.
In her talk, Cooper discussed some of the issues such as food safety that she and her team currently address. Some of the other issues discussed included food packaging, nutrition, weight, and of course variety.
Cooper cited that the current daily allocation of food for manned spaceflight crews is just under four pounds per day. Estimating a five-year trek to Mars would require over 7,000 pounds of food per crew person. “That’s a clear impediment to a lot of mission scenarios,” Cooper said. “We need new approaches. Right now, we are looking at the possibility of implementing a bioregenerative system that would involve growing crops in space and possibly shipping some bulk commodities to a Mars habitat as well. This scenario involves much more food processing and meal preparation than the current food system developed for the space shuttles and the International Space Station.” Various examples of encapsulated space food. Image Credit: NASA/Johnson Space Flight Center
The idea behind bioregenerative systems is that plants could multi-task, not only providing food, but also removing carbon dioxide gas and releasing oxygen, just like plants on Earth. Plants that are prime candidates for a Mars mission would have very little inedible structure. So far, ten plants that require little room and grow with minimal work have been identified. A few of the ten ideal plants identified are lettuce, spinach, carrots, tomatoes, strawberries, some herbs and cabbage.
One other idea Cooper suggested for future manned missions to Mars, would be to ship food products ahead of time. Sending supplies in advance of a mission would result in less food and packaging flying onboard the manned spacecraft headed to Mars. There are a few questions regarding sending supplies in advance, namely what happens if a critical supply ship fails to reach Mars and whether current food preservation technology can guarantee adequate nutritional content for a mission to Mars.
“The NASA Advanced Food Technology project is currently working to address the issues of food variety, weight, volume, nutrition and trash disposal through research and external academic and commercial collaborations,” Cooper noted.
Ray Sanders is a Sci-Fi geek, astronomer and space/science blogger. Visit his website Dear Astronomer and follow on Twitter (@DearAstronomer) or Google+ for more space musings.
Opportunity investigates Tisdale 2 rock showing indications of ancient Martian water flow. NASA's Mars Exploration Rover Opportunity used its front hazard-avoidance camera to take this picture showing the rover's arm extended toward a light-toned rock, "Tisdale 2," during Sol 2695 of the rover's work on Mars (Aug. 23, 2011). The composition of Tisdale 2 is unlike any rock studied by Opportunity since landing 7.5 years ago. It is about 12 inches (30 centimeters) tall. Credit: NASA/JPL-Caltech
Scientists directing NASA’s Mars Opportunity rover gushed with excitement as they announced that the aging robot has discovered a rock with a composition unlike anything previously explored on the Red Planet’s surface – since she landed on the exotic Martian plains 7.5 years ago – and which offers indications that liquid water might have percolated or flowed at this spot billions of years ago.
Barely three weeks ago Opportunity arrived at the rim of the gigantic 14 mile ( 22 km) wide crater named Endeavour after an epic multi-year trek, and for the team it’s literally been like a 2nd landing on Mars – and the equivalent of the birth of a whole new mission of exploration at an entirely ‘new’ landing site.
“This is like having a brand new landing site for our veteran rover,” said Dave Lavery, program executive for NASA’s Mars Exploration Rovers at NASA Headquarters in Washington. “It is a remarkable bonus that comes from being able to rove on Mars with well-built hardware that lasts.”
Opportunity has traversed an incredible distance of 20.8 miles (33.5 km) across the Meridiani Planum region of Mars since landing on January 24, 2004 for a 3 month mission – now 30 times longer than the original warranty.
“Tisdale 2” is the name of the first rock that Opportunity drove to and investigated after reaching Endeavour crater and climbing up the rim at a low ridge dubbed ‘Cape York’.
This rock, informally named "Tisdale 2," was the first rock the NASA's Mars Rover Opportunity examined in detail on the rim of Endeavour crater. It has textures and composition unlike any rock the rover examined during its first 90 months on Mars. Its characteristics are consistent with the rock being a breccia -- a type of rock fusing together broken fragments of older rocks. Image credit: NASA/JPL-Caltech/Cornell/ASU
Endeavour’s rim is heavily eroded and discontinuous and divided into a series of segmented and beautiful mountainous ridges that offer a bonanza for science.
“This is not like anything we’ve ever seen before. So this is a new kind of rock.” said Steve Squyres, principal investigator for Opportunity at Cornell University in Ithaca, N.Y at a briefing for reporters on Sept. 1.
“It has a composition similar to some volcanic rocks, but there’s much more zinc and bromine than we’ve typically seen. We are getting confirmation that reaching Endeavour really has given us the equivalent of a second landing site for Opportunity.”
Tisdale 2 is a flat-topped rock about the size of a footstool that was blasted free by the impact that formed the tennis court sized “Odyssey” crater from which it was ejected.
“The other big take-away message, and this is to me the most interesting thing about Tisdale, is that this rock has a huge amount of zinc in it, way more zinc than we have ever seen in any Martian rock. And we are puzzling, we are thinking very hard over what that means,” Squyres speculated.
Bright veins cutting across outcrop in a section of Endeavour crater's rim called "Botany Bay" are visible in the foreground and middle distance of this view assembled from images taken by the navigation camera on Opportunity during Sol 2,681on Mars (Aug. 9, 2011). Credit: NASA/JPL-Caltech
Squyres said that high levels of zinc and bromine on Earth are often associated with rocks in contact with flowing water and thus experiencing hydrothermal activity and that the impact is the source of the water.
“When you find rocks on Earth that are rich in zinc, they typically form in a place where you had some kind of hydrothermal activity going on, in other words, you have water that gets heated up and it flows through the rocks and it can dissolve out and it can get redeposited in various places,” Squyres explained.
“So this is a clue, not definitive proof yet, but this is a clue that we may be dealing with a hydrothermal system here, we may be dealing with a situation where water has percolated or flowed or somehow moved through these rocks, maybe as vapor, maybe as liquid, don’t know yet.”
“But it has enhanced the zinc concentration in this rock to levels far in excess of anything we’ve ever seen on Mars before. So that’s the beginning of what we expect is going to be a long and very interesting story about these rocks.”
Endeavour crater was chosen three years ago as the long term destination for Opportunity because it may hold clues to a time billions and billions of years ago when Mars was warmer and wetter and harbored an environment that was far more conducive to the formation of life beyond Earth.
Endeavour Crater Panorama from Opportunity, Sol 2681, August 2011
Opportunity arrived at the rim of Endeavour on Sol 2681, August 9, 2011 and climbed up the ridge known as Cape York. Odyssey crater is visible at left. The rover has driven to Tisdale 2 rock at the outskirts of Odyssey to investigate the ejecta blocks which may hold clues to ancient water flow on Mars. Distant portions of Endeavour’s rim - as far as 13 miles away – visible in the background. The rover will likely drive eventually to the Cape Tribulation rim segment at right which holds a mother lode of clay minerals. This photo mosaic was stitched together from raw images taken by Opportunity on Sol 2681.
Mosaic Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer
Signatures of clay minerals, or phyllosilicates, were detected at several spots at Endeavour’s western rim by observations from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) aboard NASA’s Mars Reconnaissance Orbiter (MRO).
“The motherlode of clay minerals is on Cape Tribulation. The exposure extends all the way to the top, mainly on the inboard side,” said Ray Arvidson, the rover’s deputy principal investigator at Washington University in St. Louis.
Opportunity Traverse Map: 2004 to 2011. The yellow line on this map shows where NASA's Mars Rover Opportunity has driven from the place where it landed in January 2004 -- inside Eagle crater, at the upper left end of the track -- to a point approaching the rim of Endeavour crater. The map traces the route through the 2,670th Martian day, or sol, of Opportunity's work on Mars (July 29, 2011). Image credit: NASA/JPL-Caltech/MSSS/NMMNHS.
Phyllosilicates are clay minerals that form in the presence of pH neutral water and which are far more hospitable to the possible genesis of life compared to the sulfate rich rocks studied in the more highly acidic aqueous environments examined by both the Opportunity and Spirit rovers thus far.
“We can get up the side of Cape Tribulation,” said Arvidson. It’s not unlike Husband Hill for Spirit. We need to finish up first at Cape York, get through the martian winter and then start working our way south along Solander Point.
The general plan is that Opportunity will probably spend the next several months exploring the Cape York region for before going elsewhere. “Just from Tisdale 2 we know that we have something really new and different here,” said Squyres.
“On the final traverses to Cape York, we saw ragged outcrops at Botany Bay unlike anything Opportunity has seen so far, and a bench around the edge of Cape York looks like sedimentary rock that’s been cut and filled with veins of material possibly delivered by water,” said Arvidson. “We made an explicit decision to examine ancient rocks of Cape York first.”
So far at least the terrain at Cape York looks safe for driving with good prospects for mobility.
Opportunity approaches Tisdale 2 rock at Endeavour Crater rim
Opportunity Mars rover climbed up the ridge known as Cape York and drove to the flat topped Tisdale 2 rock at upper left to analyze it with the science instruments on the robotic arm. This photo mosaic was stitched together from raw images taken by Opportunity on Sol 2685, August 2011.
Mosaic Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer
“The good news is that, as predicted, we have hard packed soils like the plains at Gusev that Spirit saw before getting to the Columbia Hills,” said Arvidson. “The wheel tracks at Cape York are very, very shallow. So if anything we will have some skid going downhill the slopes of 5 to 10 degrees on the inboard side which we can correct for.”
“We are always on the lookout for sand traps. We are particularly sensitized to that after the Spirit situation. So far it’s clear sailing ahead.”
Opportunity will then likely head southwards towards an area dubbed “Botany Bay” and eventually drive some 1.5 km further to the next ridge named Cape Tribulation and hopefully scale the slopes in an uphill search for that mother lode of phyllosilicates.
“My strong hope – if the rover lasts that long – is that we will have a vehicle that is capable of climbing Cape Tribulation just as we climbed Husband Hill with Spirit. So it’s obvious to try if the rover is capable, otherwise we would try something simpler. But even if we lose a wheel we still have a vehicle capable of a lot of science,” Squyres emphasized. “Then we would stick to lower ground and more gently sloping stuff.”
“The clear intention as we finish up at Cape York, and look at what to do next, is that we are going to work our way south. We will focus along the crater’s rim. We will work south along the rim of Endeavour unless some discovery unexpectedly causes us to do something else.”
“We will go where the science takes us !” Squyres stated.
Opportunity is in generally good health but the rover is showing signs of aging.
“All in all, we have a very senior rover that’s showing her age, she has some arthritis and some other issues but generally, she’s in good health, she’s sleeping well at night, her cholesterol levels are excellent and so we look forward to productive scientific exploration for the period ahead,” said John Callas, project manager for Opportunity at NASA’s Jet Propulsion Laboratory in Pasadena, Calif.
“This has the potential to be the most revealing destination ever explored by Opportunity,” said Lavery. “This region is substantially different than anything we’ve seen before. We’re looking at this next phase of Opportunity’s exploration as a whole new mission, entering an area that is significantly different in the geologic context than anything we’ve seen with the rovers.”
This image taken from orbit shows the path of the path driven by NASA's Mars Exploration Rover Opportunity in the weeks around the rover's arrival at the rim of Endeavour crater. The sol number (number of Martian days since the rover landed on Mars) are indicated along the route. Sol 2674 corresponds to Aug. 2, 2011; Sol 2688 corresponds to Aug. 16, 2011. Image credit: NASA/JPL-Caltech/University of ArizonaElevated Zinc and Bromine in Tisdale 2 Rock on Endeavour Rim. This graphic presents information gained by examining part of the Martian rock called "Tisdale 2" with the alpha particle X-ray spectrometer on Mars rover Opportunity and comparing the composition measured there with compositions of other targets examined by Opportunity and its rover twin, Spirit. The comparison targets are soil in Gusev crater, examined by Spirit; the relatively fresh basaltic rock Adirondack, examined by Spirit; the stony meteorite Marquette examined by Opportunity; and Gibraltar, an example of sulfate-rich bedrock examined by Opportunity. The target area on Tisdale 2, called "Timmins 1," contains elevated levels of bromine (Br), zinc (Zn), phosphorus (P), sulfur (S) and chlorine (Cl) relative to the non-sulfate-rich comparison rocks, and high levels of zinc and phosphorus relative to Gibraltar. Credit: NASA/JPL-Caltech/Cornell/Max Planck Institute/University of Guelph
2 billion years ago Mars may have featured a frigid ocean. Credit: Taylor Perron/UC Berkeley.
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Many planetary scientists suspect that Mars, now cold and very dry, once had a liquid water ocean covering parts of its surface. But this does not necessarily mean that the Red Planet was ever a tropical paradise… a recent paper by a team of astrobiologists suggests that Mars was much more bitter than balmy.
Astrobiologist Alberto Fairyn and colleagues have published a paper in the journal Nature Geoscience suggesting that the marked absence of phyllosilicates in Mars’ northern lowlands is indicative of a cold ocean environment, with perhaps even a boundary of frozen glaciers.
Phyllosilicates are minerals that, on Earth, are found readily in marine sediments and sedimentary rock that was formed in the presence of an ocean environment. These same minerals have also been seen via orbiting spacecraft spectrometers to be present in sediments located in Mars’ equatorial regions, but not in the northern latitudes. Fairyn and his team, intrigued by the disparity between existing models that described Mars as being once warm and wet and the lack of phyllosilicates in the north, used new climatic and geochemical models to deduce that Mars’ northern oceans must have been consistently near freezing, with portions even covered over by ice.
The current presence of moraines in the northern highlands also suggests that glaciers may have surrounded these frigid seas, which may have prevented the transportation of phyllosilicates down to the northern ocean basin. Again, to use our own planet as an analogy, moraines are rocky debris left over from the movement of glaciers. Their existence on Mars strongly suggests a period of early glaciation.
The research by Fairyn et al. contradict – or, more aptly, combine – two leading concepts of early Mars: one, that it was cold and dry and the existence of any liquid water was restricted to the equator for small periods of time; and two, that it was once globally warmer and wetter and sustained rivers, lakes and oceans of liquid water for extended periods.
Thus a cold Mars with an Arctic, icy ocean seems to be a more fitting causation of the current state of the planet, suggests Fairyn.
More research is planned, including running through more low-temperature models and hunting for ancient coastal areas that may have been impacted by icebergs. This will no doubt prove to be a challenge since much of the evidence is now buried deep beneath newer sediments and volcanic deposits. Still, Fairyn is confident that his model may help solve a long-standing debate over the history of the Red Planet.
Jason Major is a graphic designer, photo enthusiast and space blogger. Visit his website Lights in the Dark and follow him on Twitter @JPMajor or on Facebook for the most up-to-date astronomy awesomeness!
A 'rock garden' around the rim of Endeavour Crater, as seen by the Opportunity rover. Credit: NASA/JPL/Caltech; 3-D by Stu Atkinson
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Want to experience a “you-are-there” moment with the Opportunity rover on Mars? Grab a set of 3-D glasses (red/blue) and take a gander at one of the latest views from Oppy as she starts her explorations around the rim of Endeavour Crater. This stunning 3-D version of an image taken by the rover was created by our pal Stu Atkinson. This “rock garden,” as the folk from Unmanned Spaceflight are calling it, provides a view unlike anything either Mars rover has investigated yet on Mars. The region is called “Spirit Point” in honor of the now-silent rover that sits on the other side of Mars. This is actually an ejecta field of rocks thrown about after the impact that created this huge crater where the rover is now traversing, and is an exciting region for the MER scientists to explore. As Stu so poetically says in his Road to Endeavour blog, it’s also exciting because Opportunity “was sent to Mars to look at rocks, to drive between rocks, to trundle over powdery, cinnamon-hued dust that used to be rocks to get to younger, more solid rocks.”
Oppy’s found a veritable treasure trove of interesting rocks to explore, and Stu has also put together a collection of some of the most interesting in the rover’s current field of view:
The Rocks of Spirit Point. Images: NASA/JPL/Caltech; collection by Stu Atkinson
The latest mission update for Opportunity on the Mars Rover website says the rover has now reached the rock named Tinsdale 2, started a multi-sol, multi-target in-situ (contact) investigation with a Microscopic Imager (MI) mosaic of a set of surface targets collectively named “Timmins,” followed by a placement of the Alpha Particle X-ray Spectrometer (APXS) for an overnight integration. So, she is putting all her resources to work to find out more about this interesting rock.
Here’s a non-3-D, raw image of the region from Opportunity:
Opportunity's view of Endeavour Crater on sol 2696, from the navigation camera. Credit: NASA/JPL/Caltech.
Thanks to Stu for sharing his great images, and you can read more about this interesting spot on Mars in Stu’s article, “In Praise of Rock“
Endeavour Crater Panorama from Opportunity, Sol 2681, August 2011. NASA’s Opportunity Mars rover arrived at the rim of huge Endeavour crater on Sol 2681, August 9, 2011 and climbed up the ridge known as Cape York. A small crater dubbed ‘Odyssey’ is visible in the foreground at left. The rover has now driven to the outskirts of Odyssey to investigate the ejecta blocks which may stem from an ancient and wetter Martian Epoch. Opportunity snapped this soaring panorama showing distant portions of Endeavour’s rim - as far as 13 miles away - in the background. This photo mosaic was stitched together from raw images taken by Opportunity on Sol 2681. Mosaic Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer
[/caption]NASA’s Mars Opportunity rover has finally arrived at the huge Martian crater named Endeavour that simultaneously offers a mother lode of superb scenery and potentially the “Mother of all Martian Science”. The epic journey took nearly three years.
The intrepid robogirl is now climbing uphill on a Scientific quest that may well produce bountiful results towards the most important findings ever related to the search for life on Mars. Opportunity arrived at the western rim of the 13 mile (21 km) wide Endeavour crater on the 2681st Sol , or Martian day, of a mission only warrantied to last 90 Sols.
See our new Opportunity panoramic mosaics (Marco Di Lorenzo & Ken Kremer) illustrating the magnificent scenery and science targets now at hand on the surface of the Red Planet, thanks to the diligent work of the science and engineering teams who created the twin Mars Exploration Rover (MER) vehicles – Spirit & Opportunity.
Opportunity made landfall at Endeavour at a ridge of the discontinuous crater rim named Cape York and at a spot dubbed “Spirit Point” – in honor or her twin sister Spirit which stopped communicating with Earth about a year ago following more than six years of active science duty. See traverse map mosaic.
The martian robot quickly started driving northwards up the gnetle slopes of Cape York and has reached a small crater named “Odyssey” – the first science target, Dr. Matt Golembek told Universe Today. Golembek is a Senior Research Scientist with the Mars Exploration Program at the Jet Propulsion Laboratory (JPL) in Pasadena, Calif.
“Large ejecta blocks are clearly visible on the rim of Odyssey crater,” said Golembek. The crater is about 66 feet (20 m) in diameter.
Odyssey is a small impact crater of interest to the team because it features exposed material from Mars ancient Noachian era that was ejected when the crater was excavated long ago. Opportunity carefully drove over several days to one of those ejecta blocks – a flat topped rock nicknamed Tisdale 2.
Endeavour Crater Panorama from Opportunity, Sol 2685, August 2011
NASA’s Opportunity Mars rover arrived at the rim of huge Endeavour crater on Sol 2681, August 9, 2011 and is climbed up the ridge known as Cape York. She drove to the flat topped Tisdale 2 rock at upper left to analyze it with the science instruments on the robotic arm. Opportunity snapped this soaring panorama showing distant portions of Endeavour’s rim - as far as 13 miles away - in the background. This photo mosaic was stitched together from raw images taken by Opportunity on Sol 2685.
Mosaic Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer
“Opportunity is at a block of Odyssey crater ejecta called Tisdale 2 and the rock appears different from anything else we have seen,” Golembek explained.
Starting on Sol 2688 (Aug. 16) the rover began a science campaign time to investigate the rock with the instruments at the terminus of its robotic arm or IDD (Instrument Deployment Device) that will continue for some period of time.
“We are about to start an IDD campaign,” Golembek stated.
The Long Journey of Opportunity form Eagle to Endeavour Crater (2004 to 2011).
This map mosaic shows Opportunity’s epic trek of nearly eight years from landing at Eagle crater on January 24, 2004 to arrival at the giant 13 mile (21 km) diameter Endeavour crater in August 2011. Opportunity arrived the Endeavour’s rim and then drove up a ridge named Cape York. The photomosaic at top right show the outlook from Cape York on Sol 2685 (August 2011).
Mosaic Credit: NASA/JPL/Cornell/Kenneth Kremer/Marco Di Lorenzo
The team reports that the soil at Cape York is also of a different texture than any that Opportunity has seen so far on her incredible 20 mile (33 km) trek across the Meridiani Planum region of Mars. So far they haven’t seen of the iron-rich concretions, nicknamed “blueberries,” which have been plentiful on the surface along the way at numerous locations Opportunity has stopped at and investigated over the past 90 months. Initially the prime mission was projected to last 3 months – the remainder has been a huge bonus.
The science team is directing Opportunity to hunt for clay minerals, also known as phyllosilicates, that could unlock the secrets of an ancient Epoch on Mars stretching back billions and billions of years ago that was far wetter and very likely more habitable and welcoming to life’s genesis.
Phyllosilicate minerals form in neutral water that would be vastly more friendly to any potential Martian life forms – if they ever existed in the past or present. Signatures for phyllosilicates were detected by the CRISM instrument aboard NASA’s powerful Mars Reconnaissance Orbiter (MRO) spacecraft circling Mars
Flat-topped Tisdale 2 rock. Credit: NASA/JPL-Caltech'Ridout' Rock on Rim of Odyssey Crater. Opportunity looked across small Odyssey crater on the rim of much larger Endeavour crater to capture this raw image from its panoramic camera during the rover's 2,685th Martian day, or sol, of work on Mars (Aug. 13, 2011). From a position south of Odyssey, this view is dominated by a rock informally named "Ridout" on the northeastern rim of Odyssey. The rock is roughly the same size as the rover, which is 4.9 feet (1.5 meters) long. Credit: NASA/JPL-Caltech/Cornell/ASU
Kick back and watch the clouds go by — on Mars! Emily Lakdawalla at the Planetary Society Blog has put together a very nifty video from Mars Express data, showing clouds in motion over Mars. Emily has just learned a new technique called ‘tweening’ to create smooth animation videos from a series of images that are not at a very high frame rate. She explains more about the technique on her blog post here and has promised a two-part “how to” explainer for those interested in learning how to do this for yourself.
The cloudy area shown on Mars is within Noachis Terra to the west of Hellas basin, around 45 degrees south, 38 east.
Collapse pit on Mars reveals opening to an underground cave
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What would make a great home for a giant Martian ant lion? I’d have to say this pit, imaged by the HiRISE camera aboard the Mars Reconnaissance Orbiter!
Earlier this year a crater was spotted with a dark spot at its center. When the team took a closer look with the high-resolution camera they saw that the spot is actually a 35-meter (115-foot) -wide skylight that opens into an underground cavern. The cavern is most likely a section of an empty lava tube, leftovers from ancient Martian volcanic activity.
Detail of the skylight
Based on the shadows it’s estimated that the pit is about 20 meters (65 feet) deep. But, how much of that is material piled up on the floor of the cavern from the surrounding crater itself? And what caused the crater to form in the first place? These are questions that remain to be answered.
The HiRISE image itself is false-color, the hues denoting the texture and composition of the surface material and not the actual color as would be seen in visible light.
As far as a giant Martian ant lion… well, unless there are some giant Martian ants around for it to snack on, I’m going to assume there’s nobody home!
Phobos, one of the two natural satellites of Mars silhouetted against the Martian surface. Credit: ISRO
Mars Express images of Phobos from January 9, 2011 flyby
If someone were to ask you when fear was first discovered, you could tell them August 11, 1877. That’s when, 134 years ago today, Asaph Hall identified Phobos, the larger of Mars’ two moons. But even though it’s named after the Greek god of fear, there’s nothing to be afraid of…
